posted on 2019-05-09, 12:39authored byBrandon Zoellner, Shaun O’Donnell, Zongkai Wu, Dominique Itanze, Abigail Carbone, Frank E. Osterloh, Scott Geyer, Paul A. Maggard
A family of solid
solutions, Cu5(Ta1–xNbx)11O30 (0 ≤ x ≤ 0.4), was investigated as p-type semiconductors
for their band gaps and energies and for their activity for the reduction
of water to molecular hydrogen. Compositions from 0 to 40 mol % niobium
were prepared in high purity by solid-state methods, accompanied by
only very small increases in the lattice parameters of ∼0.05%
and with the niobium and tantalum cations disordered over the same
atomic sites. However, an increasing niobium content causes a significant
decrease in the bandgap size from ∼2.58 to ∼2.05 eV
owing to the decreasing conduction band energies. Linear-sweep voltammetry
showed an increase in cathodic photocurrents with niobium content
and applied negative potential of up to −0.6 mA/cm2 (pH ∼7.3; AM 1.5 G light filter with an irradiation intensity
of ∼100 mW/cm2). The cathodic photocurrents could
be partially stabilized by heating the polycrystalline films in air
at 550 °C for 1 h to produce surface nanoislands of CuO or using
protecting layers of aluminum-doped zinc oxide and titania. Aqueous
suspensions of the Cu5(Ta1–xNbx)11O30 powders were also found to be active for hydrogen production under
visible-light irradiation in a 20% aqueous methanol solution with
the highest apparent quantum yields for the 10% and 20% Nb-substituted
samples. Electronic structure calculations show that the increased
photocurrents and hydroen evolution activities of the solid solutions
arise near the percolation threshold of the niobate/tantalate framework
wherein the Nb cations establish an extended −O–Nb–O–Nb–O–
diffusion pathway for the minority carriers. The latter also reveals
a novel pathway for enhancing charge separation as a function of the
niobium–oxide connectivity. Thus, these results illustrate
the advantages of using solid solutions to achieve the smaller bandgap
sizes and band energies that are needed for solar-driven photocatalytic
reactions.